Observation details report
Detailed source parameters (including errors) in a comma-separated values file
Click on source number for detailed analysis, including spectral fits if applicable
| data | idnum | idradec | telescope | instrument | x | y | cnts | cntserr | rate | rateerr | SNR | poisprob | sigmaj | sigmin | incang | offax | cnts_soft | cnts_hard | hr | hr_err | ext | var | N_H | flux | vign | flags | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Report | srcpi bgdpi arf rmf | 1 | X183208.91-093904.5 | xmm | pn | 284.31 | 279.049 | 4228.95 | 75.0131 | 0.269481 | 0.00478006 | 147.171 | 1 | 6.0348 | 5.79801 | 71.0416 | 1.74095 | 1195.33 | 4061.46 | 0.545223 | 0.0161855 | F | F | 1.55e+22 | 1.91503e-12 | 1 | dsx |
| Report | srcpi bgdpi arf rmf | 3 | X183208.94-093904.3 | xmm | mos1 | 284.207 | 279.098 | 1824.97 | 50.839 | 0.100214 | 0.00279172 | 89.0634 | 1 | 5.31133 | 5.31133 | 0 | 1.7435 | 528.189 | 1813.85 | 0.548949 | 0.0243939 | F | F | 1.55e+22 | 1.82765e-12 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X183208.92-093903.9 | xmm | mos2 | 284.251 | 279.071 | 2604.67 | 54.0354 | 0.143045 | 0.00296756 | 180.894 | 1 | 10.875 | 10.875 | 0 | 1.74038 | 621.349 | 1998.15 | 0.525597 | 0.0233252 | F | T | 1.55e+22 | 2.59851e-12 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X183232.49-094143.2 | xmm | mos2 | 204.134 | 242.305 | 105.276 | 13.1552 | 0.00578165 | 0.00072247 | 16.2982 | 1 | 10.875 | 10.875 | 0 | 7.95644 | 82.2787 | 13.1124 | -0.72508 | 0.164512 | F | F | 1.52e+22 | 1.83321e-13 | 1 | dbx |
| Report | srcpi bgdpi arf | 1 | X183232.43-094143.1 | xmm | mos1 | 204.347 | 242.778 | 124.294 | 13.6392 | 0.00682535 | 0.000748972 | 21.0982 | 1 | 10.875 | 10.875 | 0 | 7.92568 | 98.0043 | 22.5829 | -0.625451 | 0.131163 | F | F | 1.52e+22 | 1.97558e-13 | 1 | dpbx |
| Report | srcpi bgdpi arf | 2 | X183226.59-093519.4 | xmm | pn | 224.179 | 330.698 | 89.1273 | 15.5172 | 0.00567946 | 0.000988804 | 8.10675 | 1 | 10.875 | 10.875 | 0 | 5.86983 | 83.6057 | 3.23772 | -0.925436 | 0.237013 | F | T | 1.54e+22 | 4.9267e-14 | 1 | dpx |
| Report | srcpi bgdpi arf rmf | 3 | X183232.36-094143.0 | xmm | pn | 204.573 | 242.598 | 271.795 | 22.917 | 0.0173196 | 0.00146034 | 9.45866 | 1 | 6.72002 | 4.8636 | 45.0934 | 7.91552 | 225.65 | 13.4306 | -0.887648 | 0.0993453 | F | F | 1.52e+22 | 1.90966e-13 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X183155.44-094702.9 | xmm | mos1 | 330.076 | 169.034 | 53.7041 | 11.2835 | 0.00294906 | 0.000619611 | 7.49836 | 1 | 10.875 | 10.875 | 0 | 9.65808 | -0.795622 | 49.6341 | 1 | 0.313421 | F | T | 1.53e+22 | 1.01422e-13 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X183235.96-094724.4 | xmm | mos2 | 192.39 | 164.112 | 19.9892 | 10.0826 | 0.00109778 | 0.000553723 | 2.2119 | 0.983465 | 3.36264 | 3.36264 | 0 | 12.3985 | 2.51818 | 17.5182 | 0.748639 | 0.380248 | F | F | 1.5e+22 | 9.64808e-14 | 1 | dsx |
counts and rate are bgd.-subtracted, based on simple spatial fitting (if done) or extracted counts from aperture otherwise (N.B., in either case aperture counts are given csv file).
cntserr, rateerr = Error on (source) counts and count rate, based on error in total counts
SNR = signal-to-noise ratio, computed using Nsrc/sqrt(Nbgd)
poisprob = Poisson probability of observing total counts given bgd. counts
sigmaj, sigmin = source extent (from detection output or spatial fitting) in units of arcsecs.
incang = position angle of source (inclination from x-axis)
cnts_soft = bgd.-subtracted counts in soft band (0.50 - 2.00 KeV, always taken directly from source aperture rather than model fitting)
cnts_hard = bgd.-subtracted counts in hard band (2.00 - 10.00 KeV, always taken directly from source aperture rather than model fitting)
hr, hr_err = hardness ratio ([cnts_hard-cnts_soft]/[cnts_hard+cnts_soft]) and error
ext = source extension flag: F = false (not extended), A = true (extended), A = asymetric (ratio of sigmaj/sigmin > 1 + x, where x = 0.5 by default)
var = variability flag: U = unknown, F = false (is not variable), T = true
N_H = Galactic column density as determined from LHEASOFT nh program
flux = flux determined from count rate using pimms (in the 0.30-8.00 keV bandpass for a power-law model with ph. index = 1.8)
vign = vignetting correction
Flags: d = detection parameters, s = simple spatial fitting parameters,
b = simple spatial fitting failed, p = poor simple spatial fit, x = extracted events parameters, t = temporal anaylsis parameters,
i = psf spatial fitting parameters, f = spectral fitting parameters,
c = source is confused, u = user-defined source, v = detected source coincident with user-defined source, r = source is in region-of-interest